Physical Basis of the Transport and Composition of Cosmic Rays in the Galaxy

Details Physical Basis of the Transport and Composition of Cosmic Rays in the Galaxy Physical Basis of the Transport and Composition of Cosmic Rays in the Galaxy

Jun 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrvl..22.1448g&link_type=abstract

Physical Review Letters, vol. 22, Issue 26, pp. 1448-1453

Physics

27

Scientific paper

Consideration of cosmic-ray propagation leads naturally to an equilibrium model for cosmic-ray origin and storage in the galaxy. In this model the relative abundances of nuclei with substantially different charge values are nearly energy independent. We conclude that this simple, one-"component" model is consistent with observations of both the galactic primary (i.e., H1, He4, C, N, O, Fe) and secondary particles (He3, Li, Be, B).

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